Wikipedia:Peer review/Type Ib and Ic supernovae/archive1
This peer review discussion has been closed.
I've listed this article for peer review because I was thinking of making this at least a GA. The problem is that I don't know what is there missing from this article. At this point I do not care about c/e issues or MOS, I just want to know what is not already in the article but should be in it.
Thanks, Nergaal (talk) 05:32, 8 September 2008 (UTC)
- In addition to more on the WR-SN connection, I'd like to see information on other mechanisms to produce the precursor. For example, atmospheric stripping through mass transfer in close binary systems (perhaps as a result of binary system evolution). Another example is WD-WD mergers, which may cause type Ib/Ic and type II SN. Thanks.—RJH (talk) 21:28, 8 September 2008 (UTC)